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topline=true, % colored bar at the top of the frame + topline=true, % colored bar at the top of the frame shadow=false, % Shading for beamer blocks watermark=BG_lower, % png file for the watermark ]{Flip} %\logo{\kern+1.em\includegraphics[height=1cm]{SHiP-3_LightCharcoal}} - + \usepackage[lf]{berenis} \usepackage[LY1]{fontenc} @@ -21,7 +21,7 @@ \usepackage{emerald} \usefonttheme{professionalfonts} -\usepackage[no-math]{fontspec} +\usepackage[no-math]{fontspec} \defaultfontfeatures{Mapping=tex-text} % This seems to be important for mapping glyphs properly \setmainfont{Gillius ADF} % Beamer ignores "main font" in favor of sans font @@ -63,10 +63,10 @@ \usepackage{subfigure} \usepackage{tikz} -%\usepackage{hepparticles} -\usepackage[italic]{hepparticles} +%\usepackage{hepparticles} +\usepackage[italic]{hepparticles} -\usepackage{hepnicenames} +\usepackage{hepnicenames} % Drawing a line \tikzstyle{lw} = [line width=20pt] @@ -113,10 +113,10 @@ bigvector/.style={decorate, decoration={snake,amplitude=4pt}, draw}, } -% TIKZ - for block diagrams, +% TIKZ - for block diagrams, % from http://www.texample.net/tikz/examples/control-system-principles/ % \usetikzlibrary{shapes,arrows} -\tikzstyle{block} = [draw, rectangle, +\tikzstyle{block} = [draw, rectangle, minimum height=3em, minimum width=6em] @@ -162,7 +162,7 @@ } \newcommand{\backupend}{ \addtocounter{framenumberappendix}{-\value{framenumber}} - \addtocounter{framenumber}{\value{framenumberappendix}} + \addtocounter{framenumber}{\value{framenumberappendix}} } @@ -189,8 +189,8 @@ \newcommand{\re}{{\rm Re}} \newcommand{\invfb}{\rm{fb^{-1}}} \newcommand{\fixme}{\rm{{\color{red}{FIXME!}}}} -\newcommand{\thetal}{\theta_l} -\newcommand{\thetak}{\theta_k} +\newcommand{\thetal}{\theta_l} +\newcommand{\thetak}{\theta_k} \newcommand{\nn}{\nonumber} \newcommand{\eq}[1]{\begin{equation} #1 \end{equation}} %\newcommand{\eqn}[1]{\begin{displaymath} #1 \end{displaymath}} @@ -252,7 +252,7 @@ { \setbeamertemplate{sidebar right}{\llap{\includegraphics[width=\paperwidth,height=\paperheight]{bubble2}}} -\begin{frame}[c]%{\phantom{title page}} +\begin{frame}[c]%{\phantom{title page}} \begin{center} \begin{center} \begin{columns} @@ -295,9 +295,9 @@ \item LHCb measurements of $\Pbeauty \to \Pstrange \ell \ell$. \item Global fit to $\Pbeauty \to \Pstrange \ell \ell$ measurements. \item Conclusions. -\end{enumerate} - - +\end{enumerate} + + \end{minipage} \vspace*{2.cm} \end{frame} @@ -391,7 +391,7 @@ \item Weak neutral currents were first, introduced in 1958 by Buldman. \item Later on they were naturally incorporated into unification of weak and electromagnetic interactions. -\item 't Hooft proved that the GWS models was renormalizable. +\item 't Hooft proved that the GWS models was renormalizable. \item Everything was there on theory side, only missing piece was the experiment, till 1973. \end{small} @@ -446,8 +446,8 @@ \only<1>{ \begin{minipage}{\textwidth} - - + + \begin{columns} \column{0.5\textwidth} @@ -462,30 +462,30 @@ \end{description} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{CP asymmetry:}} -\begin{description} +\begin{description} \item [$\PB^{\pm} \to \Ppi^{\pm} \Pmuon \APmuon$] {~}{~}LHCb, Sep 15 \end{description} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{Isospin asymmetry:}} -\begin{description} +\begin{description} \item [$\PB \to \PK \Pmuon \APmuon$] {~}{~}{~}{~}{~}LHCb, Mar 14 \end{description} \column{0.5\textwidth} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{Lepton Universality:}} -\begin{description} +\begin{description} \item [$\PB^{\pm} \to \PK^{\pm} \Plepton \APlepton$] {~}{~}LHCb, Jun 14 \end{description} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{Angular:}} -\begin{description} +\begin{description} \item [$\PB^{0} \to \PK^{\ast} \Plepton \APlepton$] {~}{~}{~}LHCb, Jan 15 \item [$\PB^{\pm} \to \PK^{\ast,\pm} \Plepton \APlepton$] BaBar, Aug 15 \item [$\PBs \to \Pphi \Plepton \APlepton$] {~}{~}{~}LHCb, Jun 15 \item [$\PLambdab \to \PLambda \Pmuon \APmuon$] {~}{~}LHCb, Mar 15 -\end{description} +\end{description} @@ -498,8 +498,8 @@ \only<2>{ \begin{minipage}{\textwidth} - - + + \begin{columns} \column{0.5\textwidth} @@ -514,30 +514,30 @@ \end{description} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{CP asymmetry:}} -\begin{description} +\begin{description} \item [$\PB^{\pm} \to \Ppi^{\pm} \Pmuon \APmuon$] {~}{~}LHCb, Sep 15 \end{description} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{Isospin asymmetry:}} -\begin{description} +\begin{description} \item [$\PB \to \PK \Pmuon \APmuon$] {~}{~}{~}{~}{~}LHCb, Mar 14 \end{description} \column{0.5\textwidth} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{Lepton Universality:}} -\begin{description} +\begin{description} \item [{\color{red}{$\PB^{\pm} \to \PK^{\pm} \Plepton \APlepton$}}] {~}{~}{\color{red}{LHCb, Jun 14}} \end{description} $\color{JungleGreen}{\Rrightarrow}$ {\color{WildStrawberry}{Angular:}} -\begin{description} +\begin{description} \item [{\color{red}{$\PB^{0} \to \PK^{\ast} \Plepton \APlepton$}}] {~}{~}{~}LHCb, Jan 15 \item [{\color{red}{$\PB^{\pm} \to \PK^{\ast,\pm} \Plepton \APlepton$}}] {\color{red}{BaBar, Aug 15}} \item [$\PBs \to \Pphi \Plepton \APlepton$] {~}{~}{~}LHCb, Jun 15 \item [{\color{red}{$\PLambdab \to \PLambda \Pmuon \APmuon$}}] {~}{~}{\color{red}{LHCb, Mar 15}} -\end{description} +\end{description} \begin{alertblock}{} $>2~\sigma$ deviations from SM @@ -560,13 +560,13 @@ \begin{columns} \column{0.6\textwidth} August 2013:\\ - + \includegraphics[width=0.95\textwidth]{images/P5prime.png} \column{0.4\textwidth} \begin{itemize} \item LHCb observed a deviation in $4.3-8.68~\GeV^2$ using $1~\invfb$ of data. \item It turned out that the discrepancy occurred in an observable that was not constrained. -\item $q^2$ is the dimuon invariant mass. +\item $q^2$ is the dimuon invariant mass. \end{itemize} \end{columns} @@ -583,12 +583,12 @@ \begin{columns} \column{0.6\textwidth} August 2013:\\ - + \includegraphics[width=0.95\textwidth]{images/P5prime.png} \column{0.4\textwidth} \begin{itemize} \item LHCb observed a deviation in $4.3-8.68~\GeV^2$ using $1~\invfb$ of data. -\item It turned out that the discrepancy occurred in an observable that was not constrained. +\item It turned out that the discrepancy occurred in an observable that was not constrained. \end{itemize} \end{columns} @@ -611,38 +611,38 @@ {~} \begin{minipage}{\textwidth} -\begin{itemize} -\item \textbf{Operator Product Expansion and Effective Field Theory} -\end{itemize} -\begin{columns} -\column{0.1in}{~} -\column{3.2in} +\begin{itemize} +\item \textbf{Operator Product Expansion and Effective Field Theory} +\end{itemize} +\begin{columns} +\column{0.1in}{~} +\column{3.2in} \begin{footnotesize} -\begin{align*} +\begin{align*} H_{eff} = - \dfrac{4G_f}{\sqrt{2}} V V^{\prime \ast}\ \sum_i \left[\underbrace{C_i(\mu)O_i(\mu)}_\text{left-handed} +\ -\underbrace{C'_i(\mu)O'_i(\mu)}_\text{right-handed}\right], -\end{align*} +\underbrace{C'_i(\mu)O'_i(\mu)}_\text{right-handed}\right], +\end{align*} \end{footnotesize} -\column{2in} -\begin{tiny} -\begin{description} - \item[i=1,2] Tree - \item[i=3-6,8] Gluon penguin - \item[i=7] Photon penguin - \item[i=9.10] EW penguin - \item[i=S] Scalar penguin - \item[i=P] Pseudoscalar penguin - \end{description} - -\end{tiny} -\end{columns} -where $C_i$ are the Wilson coefficients and $O_i$ are the corresponding effective operators. -\begin{center} -\includegraphics[width=0.85\textwidth,height=3cm]{images/all.png} - -\end{center} +\column{2in} +\begin{tiny} +\begin{description} + \item[i=1,2] Tree + \item[i=3-6,8] Gluon penguin + \item[i=7] Photon penguin + \item[i=9.10] EW penguin + \item[i=S] Scalar penguin + \item[i=P] Pseudoscalar penguin + \end{description} + +\end{tiny} +\end{columns} +where $C_i$ are the Wilson coefficients and $O_i$ are the corresponding effective operators. +\begin{center} +\includegraphics[width=0.85\textwidth,height=3cm]{images/all.png} + +\end{center} @@ -657,11 +657,11 @@ \begin{frame}{$\PBzero \to \PKstar \Pmuon \APmuon$ kinematics} {~} \begin{minipage}{\textwidth} - + $\color{JungleGreen}{\Rrightarrow}$ The kinematics of $\PBzero \to \PKstar \Pmuon \APmuon$ decay is described by three angles $\thetal$, $\thetak$, $\phi$ and invariant mass of the dimuon system ($q^2)$. - - \only<1>{ -\begin{columns} + + \only<1>{ +\begin{columns} \column{0.5\textwidth} $\color{JungleGreen}{\Rrightarrow}$ $\cos \thetak$: the angle between the direction of the kaon in the $\PKstar$ ($\overline{\PKstar}$) rest frame and the direction of the $\PKstar$ ($\overline{\PKstar}$) in the $\PBzero$ ($\APBzero$) rest frame.\\ @@ -676,12 +676,12 @@ \end{columns} } \only<2>{ -{\tiny{ +{\tiny{ \eqa{\label{dist} \frac{d^4\Gamma}{dq^2\,d\!\cos\theta_K\,d\!\cos\theta_l\,d\phi}&=&\frac9{32\pi} \bigg[ J_{1s} \sin^2\theta_K + J_{1c} \cos^2\theta_K + (J_{2s} \sin^2\theta_K + J_{2c} \cos^2\theta_K) \cos 2\theta_l\nn\\[1.5mm] &&\hspace{-2.7cm}+ J_3 \sin^2\theta_K \sin^2\theta_l \cos 2\phi + J_4 \sin 2\theta_K \sin 2\theta_l \cos\phi + J_5 \sin 2\theta_K \sin\theta_l \cos\phi \nn\\[1.5mm] -&&\hspace{-2.7cm}+ (J_{6s} \sin^2\theta_K + {J_{6c} \cos^2\theta_K}) \cos\theta_l +&&\hspace{-2.7cm}+ (J_{6s} \sin^2\theta_K + {J_{6c} \cos^2\theta_K}) \cos\theta_l + J_7 \sin 2\theta_K \sin\theta_l \sin\phi + J_8 \sin 2\theta_K \sin 2\theta_l \sin\phi \nn\\[1.5mm] &&\hspace{-2.7cm}+ J_9 \sin^2\theta_K \sin^2\theta_l \sin 2\phi \bigg]\,, } @@ -742,7 +742,7 @@ \eqa{ \apeLR &=&\sqrt{2} N m_B(1- \hat s)\bigg[ (\Ceff9 + \Cpeff9) \mp (\C{10} + \Cp{10}) +\frac{2\hat{m}_b}{\hat s} (\Ceff7 + \Cpeff7) \bigg]\xi_{\bot}(E_{K^*}) \nn \\[2mm] -\apaLR &=& -\sqrt{2} N m_B (1-\hat s)\bigg[(\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10}) +\apaLR &=& -\sqrt{2} N m_B (1-\hat s)\bigg[(\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10}) +\frac{2\hat{m}_b}{\hat s}(\Ceff7 - \Cpeff7) \bigg] \xi_{\bot}(E_{K^*}) \nn \\[2mm] \azeLR &=& -\frac{N m_B (1-\hat s)^2}{2 \hat{m}_{K^*} \sqrt{\hat s}} \bigg[ (\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10}) + 2\hat{m}_b (\Ceff7 - \Cpeff7) \bigg]\xi_{\|}(E_{K^*}), \label{LargeRecoilAs}} @@ -759,51 +759,51 @@ \end{frame} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% -\begin{frame} -\only<1>{\frametitle{LHCb detector - tracking} -\begin{columns} -\column{3in} -\includegraphics[width=0.9\textwidth]{images/1050px-Lhcbview.jpg} - -\column{2in} -\includegraphics[width=0.95\textwidth]{images/sketch.png} -\end{columns} -\begin{itemize} -\item Excellent Impact Parameter (IP) resolution ($20~\rm \mu m$).\\ -$\Rightarrow$ Identify secondary vertices from heavy flavour decays -\item Proper time resolution $\sim~40~\rm fs$.\\ -$\Rightarrow$ Good separation of primary and secondary vertices. -\item Excellent momentum ($\delta p/p \sim 0.4 - 0.6\%$) and inv. mass resolution.\\ -$\Rightarrow$ Low combinatorial background. - -\end{itemize} - - -} - -\only<2>{\frametitle{LHCb detector - particle identification} -\begin{columns} -\column{3in} -\includegraphics[width=0.9\textwidth]{images/1050px-Lhcbview.jpg} - -\column{2in} -\includegraphics[width=0.95\textwidth]{images/cher.png} -\end{columns} -\begin{itemize} -\item Excellent Muon identification $\epsilon_{\mu \to \mu} \sim 97\%$, $\epsilon_{\pi \to \mu} \sim 1-3\%$ -\item Good $\PK-\Ppi$ separation via RICH detectors, $\epsilon_{\PK \to \PK} \sim 95\%$, $\epsilon_{\Ppi \to \PK} \sim 5\%$.\\ -$\Rightarrow$ Reject peaking backgrounds. -\item High trigger efficiencies, low momentum thresholds. -Muons: $p_T > 1.76 \GeV$ at L0, $p_T > 1.0 \GeV$ at HLT1,\\ -$B \to \PJpsi X $: Trigger $\sim 90\%$. - -\end{itemize} - - -} - - -\end{frame} +\begin{frame} +\only<1>{\frametitle{LHCb detector - tracking} +\begin{columns} +\column{3in} +\includegraphics[width=0.9\textwidth]{images/1050px-Lhcbview.jpg} + +\column{2in} +\includegraphics[width=0.95\textwidth]{images/sketch.png} +\end{columns} +\begin{itemize} +\item Excellent Impact Parameter (IP) resolution ($20~\rm \mu m$).\\ +$\Rightarrow$ Identify secondary vertices from heavy flavour decays +\item Proper time resolution $\sim~40~\rm fs$.\\ +$\Rightarrow$ Good separation of primary and secondary vertices. +\item Excellent momentum ($\delta p/p \sim 0.4 - 0.6\%$) and inv. mass resolution.\\ +$\Rightarrow$ Low combinatorial background. + +\end{itemize} + + +} + +\only<2>{\frametitle{LHCb detector - particle identification} +\begin{columns} +\column{3in} +\includegraphics[width=0.9\textwidth]{images/1050px-Lhcbview.jpg} + +\column{2in} +\includegraphics[width=0.95\textwidth]{images/cher.png} +\end{columns} +\begin{itemize} +\item Excellent Muon identification $\epsilon_{\mu \to \mu} \sim 97\%$, $\epsilon_{\pi \to \mu} \sim 1-3\%$ +\item Good $\PK-\Ppi$ separation via RICH detectors, $\epsilon_{\PK \to \PK} \sim 95\%$, $\epsilon_{\Ppi \to \PK} \sim 5\%$.\\ +$\Rightarrow$ Reject peaking backgrounds. +\item High trigger efficiencies, low momentum thresholds. +Muons: $p_T > 1.76 \GeV$ at L0, $p_T > 1.0 \GeV$ at HLT1,\\ +$B \to \PJpsi X $: Trigger $\sim 90\%$. + +\end{itemize} + + +} + + +\end{frame} @@ -818,7 +818,7 @@ \item PID, kinematics and isolation variables used in a Boosted Decision Tree (BDT) to discriminate signal and background. \item Reject the regions of $\PJpsi$ and $\Ppsi(2S)$. \item Specific vetos for backgrounds: $\PLambdab \to \Pproton \PK \Pmu \Pmu$, $\PBs \to \Pphi \Pmu \Pmu$, etc. -\item Using k-Fold technique and signal proxy $\PB \to \PJpsi \PKstar$ for training the BDT. +\item Using k-Fold technique and signal proxy $\PB \to \PJpsi \PKstar$ for training the BDT. \item Improved selection allowed for finer binning than the $1\invfb$ analysis. \end{itemize} @@ -896,7 +896,7 @@ \epsilon (\cos \thetal, \cos \thetak, \phi, q^2) = \\\sum_{ijkl} P_i(\cos \thetal) P_j(\cos \thetak ) P_k(\phi) P_l(q^2), \end{align*} where $P_i$ is the Legendre polynomial of order $i$. -\item We use up to $4^{th}, 5^{th}, 6^{th}, 5^{th}$ order for the $\cos \thetal, \cos \thetak, \phi, q^2$. +\item We use up to $4^{th}, 5^{th}, 6^{th}, 5^{th}$ order for the $\cos \thetal, \cos \thetak, \phi, q^2$. \end{itemize} @@ -1001,7 +1001,7 @@ \end{center} \begin{itemize} -\item Recent LHCb measurement [JHEPP09 (2015) 179]. +\item Recent LHCb measurement [JHEPP09 (2015) 179]. \item Suppressed by $\frac{f_s}{f_d}$. \item Cleaner because of narrow $\Pphi$ resonance. \item $3.3~\sigma$ deviation in SM in the $1-6\GeV^2$ bin. @@ -1017,7 +1017,7 @@ \begin{frame}{Branching fraction measurements of $\PLambdab \to \PLambda \Pmu \Pmu$} {~} \begin{minipage}{\textwidth} - + \begin{center} \only<1>{ \includegraphics[width=0.65\textwidth]{images/Lb_BR.png} @@ -1027,13 +1027,13 @@ \includegraphics[width=0.45\textwidth]{images/Lbhigh.png} } - - + + \end{center} \begin{itemize} -\item This years LHCb measurement [JHEP 06 (2015) 115]]. +\item This years LHCb measurement [JHEP 06 (2015) 115]]. \item In total $\sim 300$ candidates in data set. \item Decay not present in the low $q^2$. @@ -1075,26 +1075,26 @@ \begin{frame}{Lepton universality test} {~} \begin{minipage}{\textwidth} -\begin{columns} -\column{3.0in} -\begin{itemize} -\item If $\PZprime$ is responsible for the $P'_5$ anomaly, does it couple equally to all flavours? -\includegraphics[width=0.9\textwidth]{images/uni2.png} -\item Challenging analysis due to bremsstrahlung. -\item Migration of events modeled by MC. -\item Correct for bremsstrahlung. -\item Take double ratio with $\PBplus \to \PJpsi \PKplus$ to cancel systematics. -\item In $3\invfb$, LHCb measures $R_K=0.745^{+0.090}_{-0.074}(stat.)^{+0.036}_{-0.036}(syst.)$ -\item Consistent with SM at $2.6\sigma$. - -\end{itemize} -\column{2.0in} -\includegraphics[width=0.99\textwidth]{images/RK.png}\\ -\begin{itemize} -\item \href{http://arxiv.org/abs/1406.6482}{Phys. Rev. Lett. 113, 151601 (2014)} -\end{itemize} -\end{columns} - +\begin{columns} +\column{3.0in} +\begin{itemize} +\item If $\PZprime$ is responsible for the $P'_5$ anomaly, does it couple equally to all flavours? +\includegraphics[width=0.9\textwidth]{images/uni2.png} +\item Challenging analysis due to bremsstrahlung. +\item Migration of events modeled by MC. +\item Correct for bremsstrahlung. +\item Take double ratio with $\PBplus \to \PJpsi \PKplus$ to cancel systematics. +\item In $3\invfb$, LHCb measures $R_K=0.745^{+0.090}_{-0.074}(stat.)^{+0.036}_{-0.036}(syst.)$ +\item Consistent with SM at $2.6\sigma$. + +\end{itemize} +\column{2.0in} +\includegraphics[width=0.99\textwidth]{images/RK.png}\\ +\begin{itemize} +\item \href{http://arxiv.org/abs/1406.6482}{Phys. Rev. Lett. 113, 151601 (2014)} +\end{itemize} +\end{columns} + \end{minipage} @@ -1108,7 +1108,7 @@ \begin{frame}{Angular analysis of $\PBzero \to \PKstar \Pe \Pe$} {~} \only<1>{ - \begin{minipage}{\textwidth} + \begin{minipage}{\textwidth} \begin{itemize} \item With the full data set ($3\invfb$) we performed angular analysis in $0.0004 < q^2 <1~\GeV^2$. \item Electrons channels are extremely challenging experimentally: @@ -1121,10 +1121,10 @@ \begin{equation} \label{eq:physPars} \begin{split} - \FL &=\frac{|A_0|^2}{|A_0|^2+|A_{||}|^2 + |A_\perp|^2}\\ - \ATD &= \frac{|A_\perp|^2-|A_{||}|^2}{|A_\perp|^2+|A_{||}|^2}\\ + \FL &=\frac{|A_0|^2}{|A_0|^2+|A_{||}|^2 + |A_\perp|^2}\\ + \ATD &= \frac{|A_\perp|^2-|A_{||}|^2}{|A_\perp|^2+|A_{||}|^2}\\ \ATRe &= \frac{2\Real(A_{||L}A^*_{\perp L} + A_{||R}A^*_{\perp R})}{|A_{||}|^2 + |A_\perp|^2}\\ - \ATIm &= \frac{2\Imag(A_{||L}A^*_{\perp L} + A_{||R}A^*_{\perp R})}{|A_{||}|^2 + |A_\perp|^2}, + \ATIm &= \frac{2\Imag(A_{||L}A^*_{\perp L} + A_{||R}A^*_{\perp R})}{|A_{||}|^2 + |A_\perp|^2}, \end{split} \end{equation} @@ -1168,8 +1168,8 @@ \item Overall there is around $4.5~\sigma$ discrepancy wrt. SM. \end{itemize} - - + + \end{minipage} @@ -1187,8 +1187,8 @@ \item Overall there is around $4.5~\sigma$ discrepancy wrt. SM. \end{itemize} \includegraphics[width=0.9\textwidth]{images/C9.png} - - + + \end{minipage} @@ -1196,6 +1196,18 @@ \end{frame} + +\begin{frame}{Theory implications} +{~} + \begin{minipage}{\textwidth} + +\includegraphics[height=0.9\textheight]{images/table.png} + + +\end{minipage} + \vspace*{2.1cm} +\end{frame} + %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \begin{frame}{If not NP?} {~} @@ -1204,7 +1216,7 @@ \item We are not there yet! \item There might be something not taken into account in the theory. \item Resonances ($\PJpsi$, $\Ppsi(2S)$) tails can mimic NP effects. -\item There might be some no factorizable QCD corrections.\\ +\item There might be some non factorizable QCD corrections.\\ '' However, the central value of this effect would have to be significantly larger than expected on the basis of existing estimates'' \texttt{D.Straub, 1503.06199} . \end{itemize} @@ -1232,9 +1244,9 @@ \end{itemize} \includegraphics[width=0.9\textwidth]{images/C9_S_P.png} - + \end{minipage} - \vspace*{2.1cm} + \vspace*{2.1cm} \end{frame} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \begin{frame}{There is more!} @@ -1253,9 +1265,9 @@ \includegraphics[width=0.52\textwidth]{images/RDstar.png} -\end{center} +\end{center} \end{minipage} - \vspace*{2.1cm} + \vspace*{2.1cm} \end{frame} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% @@ -1274,9 +1286,9 @@ Standard Model explanations, whatever remains,\\ however improbable, must be New Physics.''\\ prof. Joaquim Matias - + \end{minipage} - \vspace*{2.1cm} + \vspace*{2.1cm} \end{frame} @@ -1291,22 +1303,22 @@ \includegraphics[width=0.8\textwidth]{images/Joke.jpg} \end{center} - - - + + + \end{minipage} - \vspace*{2.1cm} + \vspace*{2.1cm} \end{frame} -\backupbegin +\backupbegin \begin{frame}\frametitle{Backup} -\topline +\topline \end{frame} -\backupend +\backupend \end{document}